X-ray CCD for spectroscopy and polarization in space
X-ray CCD for spectroscopy and polarization in space
批准号:
08504001
负责人:
KOYAMA Katsuji
金额:
$44.61万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (A)
财政年份:
1996
资助国家:
日本
项目状态:
已结题
起止时间:
1996 至 1998
中文摘要
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英文摘要
The present decade is opening new frontiers in high energy astrophysics. After the X-ray satellites in the 1980's, several satellites are or will soon be simultaneously in orbit offering spectacular advances in X-ray imaging at low energiesm, as well as at high energies, in spectroscopy with increased bandwidth , and in timing. These allow us to study X-ray atomic radiation from hot plasmas (thermal X-rays) and/or high energy electrons (non-thermal X-rays). The key issue is how to separately observe the thermal and non-thermal X-rays. One typical example is found with ASCA.We discovered synchrotron X-ray emission emitted by very high energy charged particles in some supernova remnants. Subsequent observations by a Cherenkov telescope, CANGAROO, detected very high energy gamma-rays in the TeV range from one of the supernova remnants. These discoveries are clear evidences for the shock waves of the supernova remnants to be the origin of the cosmic rays.For further development to separate … More ly observe the thermal and non-thermal X-rays , we have planed to develop the technology of direct detection of X-ray polaization, coupled with imaging and spectroscopic capabilities. We have already demonstrated that a small pixel size CCD has these potentialities. We thus intended to develop small pixel size and thick depletion layer CCDs. The second requirement is also essential, because non-thermal X-rays are usually extending up to high energies.The items and results of our study are ;(1) We have made thick layer CCDs and developed the signal processing method to reduce the read-out noises.(2) We are developing 8-micron pixel CCDs to increase analizing power for the polarized X-rays(3) Since small pixel CCDs require high read-out logic, we have developed this technology(4) All above technologies are space-qualified by many environmental tests. In particular, we have studied and developed the radiation-damage-in-space and its restoration technique.(5) In parallel with these technology innovations, we have made many astrophysical studies using X-ray CCDs onboard the ASCA satellite. Less
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M.Nishiuchi: "Hard X-Ray Response of the Proto Type CCD Camera (XIS) for Astro-E" SPIE's 43rd Annual Meeting(1998),,EUV, X-Ray and Gamma-RayInstrumentation for Astronomy VIII(sd09). (1998)
M.Nishiuchi:“Astro-E 原型 CCD 相机 (XIS) 的硬 X 射线响应”SPIE 第 43 届年会(1998 年),天文学 VIII 的 EUV、X 射线和伽马射线仪器(sd09)。
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J.W.Keohane: "A Possible Site of Cosmic Ray Acceleration in the Supernova Remnant IC443" Astrophys.J.484. 350-359 (1997)
J.W.Keohane:“超新星遗迹 IC443 中宇宙射线加速的可能位置”Astrophys.J.484。
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L.Carkner,et al.: "X-Ray Emitting T-Tau i Stars in the L1551 Cloud" Astrophys.J.464. 286-305 (1996)
L.Carkner 等人:“L1551 云中的 X 射线发射 T-Tau i 恒星”Astrophys.J.464。
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K.A.Weavwer,et al.: "Iron Ka Evidence for Two X-Ray Reprocesors in MCG-5-23-16" Astrophys.J.474. 675-685 (1997)
K.A.Weavwer 等人:“MCG-5-23-16 中两个 X 射线还原机的铁 Ka 证据”Astrophys.J.474。
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T.G.Tsuru: "Cround Calibration of X-ray CCD Camera XIS onboard ASTRO-E" 32nd COSPAR Scientific Assembly, Broad Band X-Ray Spectra of Cosmic Sources, {3445-27}. (1998)
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共 30 条
Study for the Galactic Center Activity and Origin of the Highest Energy Cosmic Rays
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批准号:18204015
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项目类别:Grant-in-Aid for Scientific Research (A)
-
资助金额:$18.8万
-
财政年份:2006
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负责人:KOYAMA Katsuji
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依托单位:
High Energy Particle Acceleration at the Galactic Center Region
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批准号:13304018
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项目类别:Grant-in-Aid for Scientific Research (A)
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资助金额:$27.29万
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财政年份:2001
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负责人:KOYAMA Katsuji
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依托单位:
Study of extended X-ray sources
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批准号:02402001
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项目类别:Grant-in-Aid for General Scientific Research (A)
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资助金额:$14.14万
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财政年份:1990
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负责人:KOYAMA Katsuji
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依托单位:
海外基金